Re: [arts-users] Polarized brightness temperature

2023-10-17 Thread suifengbenpao2023
Hi Patrick,

Thank you for your quick reply, the advice you provided is very helpful, thank 
you again very much!

Best wishes,
Jiaan He
At 2023-10-18 01:11:31, "Patrick Eriksson"  
wrote: >Hi, > >The only way to get ARTS to do QV and QH automatically, is to 
use a >"system" denoted as metmm. You find it in folder > 
>arts/controlfiles/instruments/metmm > >It is not totally straightforward to 
use and the documentation is not >extensive. As far as I know, the 
documentation is basically the file >TestMetMM.arts. > >The sensor definitions 
are found in sub-folder sensor_descriptions. >Inside these QV and QH are 
denoted AMSU-V and AMSU-H. This assumes that >QH and Qv work in the same way 
for all cross-track microwave radiometer. >I assume this is true, but I am not 
100% sure. > >Bye, > >Patrick > > > >On 2023-10-17 14:15, suifengbenpao2023 
wrote: >> Dear ARTS community, >> >> >> ARTS provides calculation methods for 
vertical polarization and >> horizontal polarization. However, many sensors are 
now set up with QH >> and QV polarization. I simulated the brightness 
temperature of a >> satellite borne microwave radiometer channel at 23.8GHz (QH 
>> polarization) over the ocean using a one-dimensional atmosphere, and the >> 
first Stokes vector I obtained was close to the observed QH polarization >> 
brightness temperature. However, the simulated brightness temperature of >> H 
polarization (instrument_pol, [6] ) was significantly different from >> the 
observed QH brightness temperature, May I ask if it is possible to >> simulate 
the QH polarization of spaceborne radiometers through the H >> polarization of 
ARTS? Is it still possible that I input other variables >> incorrectly? >> >> 
>> Looking forward to your reply!Thank you! >> >> Best wishes, >> >> Jiaan He

Re: [arts-users] Polarized brightness temperature

2023-10-17 Thread Patrick Eriksson

Hi,

The only way to get ARTS to do QV and QH automatically, is to use a 
"system" denoted as metmm. You find it in folder


arts/controlfiles/instruments/metmm

It is not totally straightforward to use and the documentation is not 
extensive. As far as I know, the documentation is basically the file 
TestMetMM.arts.


The sensor definitions are found in sub-folder sensor_descriptions. 
Inside these QV and QH are denoted AMSU-V and AMSU-H. This assumes that 
QH and Qv work in the same way for all cross-track microwave radiometer. 
I assume this is true, but I am not 100% sure.


Bye,

Patrick



On 2023-10-17 14:15, suifengbenpao2023 wrote:

Dear ARTS community,


ARTS provides calculation methods for vertical polarization and 
horizontal polarization. However, many sensors are now set up with QH 
and QV polarization. I simulated the brightness temperature of a 
satellite borne microwave radiometer channel at 23.8GHz (QH 
polarization) over the ocean using a one-dimensional atmosphere, and the 
first Stokes vector I obtained was close to the observed QH polarization 
brightness temperature. However, the simulated brightness temperature of 
H polarization (instrument_pol, [6] ) was significantly different from 
the observed QH brightness temperature, May I ask if it is possible to 
simulate the QH polarization of spaceborne radiometers through the H 
polarization of ARTS? Is it still possible that I input other variables 
incorrectly?



Looking forward to your reply!Thank you!

Best wishes,

Jiaan He


[arts-users] Polarized brightness temperature

2023-10-17 Thread suifengbenpao2023
Dear ARTS community,




ARTS provides calculation methods for vertical polarization and horizontal 
polarization. However, many sensors are now set up with QH and QV polarization. 
I simulated the brightness temperature of a satellite borne microwave 
radiometer channel at 23.8GHz (QH polarization) over the ocean using a 
one-dimensional atmosphere, and the first Stokes vector I obtained was close to 
the observed QH polarization brightness temperature. However, the simulated 
brightness temperature of H polarization (instrument_pol, [6] ) was 
significantly different from the observed QH brightness temperature, May I ask 
if it is possible to simulate the QH polarization of spaceborne radiometers 
through the H polarization of ARTS? Is it still possible that I input other 
variables incorrectly?




Looking forward to your reply!Thank you!  
Best wishes,
Jiaan He